赔偿
发表于 2025-3-25 05:34:36
Razvan Solea,Daniela Cristina Cernegaxist for the majority of cool stars between the flux densities measured in the various coronal, transition-region and excess chromospheric emissions (the “flux-flux relations”). These relations do not depend on effective temperature and surface gravity..There is also a clear “activity-rotation” rela
宏伟
发表于 2025-3-25 11:09:20
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愤世嫉俗者
发表于 2025-3-25 12:14:57
Andreea Radu,Leon Rothkrantz,Mirko Novakxist for the majority of cool stars between the flux densities measured in the various coronal, transition-region and excess chromospheric emissions (the “flux-flux relations”). These relations do not depend on effective temperature and surface gravity..There is also a clear “activity-rotation” rela
可以任性
发表于 2025-3-25 16:43:47
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Glower
发表于 2025-3-25 21:08:31
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同义联想法
发表于 2025-3-26 03:25:03
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Solace
发表于 2025-3-26 07:45:51
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indicate
发表于 2025-3-26 11:36:51
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轨道
发表于 2025-3-26 15:26:19
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Detoxification
发表于 2025-3-26 17:08:10
Andrea Schirru,Simone Pampuri,Cristina De Luca,Giuseppe De Nicolaoctral types that, on the basis of current models, correspond to fully convective interiors. Hence, the results support a rotation-dependent distributed dynamo (or some variation thereof) as a viable model for the generation of magnetic flux in the very low mass stars. Future work should include v si